{"as_of":"2026-08-18T00:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:983a2a3c1887adac46936fa92143da645144a5c72afb9ecf2b16b9771d94f5ef","coverage":[{"denominator":86,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":86,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-12T01:30:43.080456Z","state":"measured"},{"denominator":86,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":86,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2607.03569/citation-record","integrity":"/paper/2607.03569/integrity","json":"/paper/2607.03569/citation-record.json","paper":"/paper/2607.03569"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Planck),H early 0 , and •late-time data (e.g","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:774b75ab3909dfc9bcd4306c268d98d69259ab021ec54ed8fb600837fd0b4bf7","observation_id":"2d4bb71b-0f88-4a87-a2b8-52ad21afc368","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"gold stand- ard","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:2fc3c7ff193cefa7103c1721ae898a0ff21eeac77fe6e1a989936c361ce11592","observation_id":"028d01cd-a64b-4ddc-a2f9-3a76572823a6","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"dilaton,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:ca2bd74c37954b7705310c0a898855b9a242508213cb0d04bfe9047adb0af176","observation_id":"7149f215-a2c7-4618-8a54-61210acad5ee","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:7f0b4b38b863c8007b1df64d9775c91e33c194c2f7a70504bb750f22e5cfe3f3","observation_id":"92befe4f-6795-4052-b5d7-3189df631bd1","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Aghanimet al.(Planck), Planck 2018 results","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:1a273bf72cda187ca2b53e9e88886be28bf89d2a009f94bdc0c9ce1c7b35efe2","observation_id":"6035183e-5144-48f0-8dea-c197b2b4857a","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:50de7161e319585f4226de4d6cb17ae37d061fe825a23902774cf0b94f651ded","observation_id":"b16f73f9-c62b-4d0c-9e52-4ae0de1f8be4","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.1955","last_updated":"2010-05-11T21:26:52Z","snapshot_observed_at":"2026-08-15T05:19:19.705098Z","submitted_at":"2010-05-11T21:26:52Z","title":"The Megamaser Cosmology Project. II. The Angular-Diameter Distance to UGC 3789","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.1955","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1005.1955","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:678fba858ce46c35346889139d50c802fc6c6d8f40c9d3562f732e2065271496","observation_id":"f2ef8b40-2857-4fc6-8f13-e6aa92861c4a","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.00017","last_updated":"2017-01-22T12:42:21Z","snapshot_observed_at":"2026-08-14T21:50:20.747348Z","submitted_at":"2016-06-30T20:00:39Z","title":"H0LiCOW I. $H_0$ Lenses in COSMOGRAIL's Wellspring: Program Overview","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.00017","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1607.00017","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:871b41b294c0491bf119284c6e1cfc5e0ef1ab08490f3908a97e24715343df61","observation_id":"15740df8-dfdb-43ca-a363-f3b7668b3815","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-08-16T02:36:16.088814Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01183","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Di Valentino, O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:dd75c97f4dcf0d2e84a780c9702f64bef5eb43ccf313c3dda0e8796551e3306f","observation_id":"3e5d5b78-2f62-4d9c-b368-1404e8905687","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.05709","last_updated":"2023-02-11T14:51:33Z","snapshot_observed_at":"2026-08-16T15:56:03.414690Z","submitted_at":"2023-02-11T14:51:33Z","title":"Hubble Tension: The Evidence of New Physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.05709","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Hu and F.-Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2302.05709","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:faa7784f872962aaf64147b6f8d1213ce1e806c48ff3130434572a5206d71c5e","observation_id":"18fe3193-25d2-4b6e-a46f-7baa99bc2253","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.01669","last_updated":"2025-08-04T13:56:55Z","snapshot_observed_at":"2026-08-13T17:48:59.058079Z","submitted_at":"2025-04-02T12:17:19Z","title":"The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.01669","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Di Valentinoet al.(CosmoVerse Network), The Cos- moVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics, Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2504.01669","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:1c014bc7f05bfa2789745b9782ee5c7de1c29ee0ddd2541ccd9098675bda76ec","observation_id":"e210d6f7-57e8-45c9-a604-36674a9fd1dd","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-15T03:29:17.716518Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.20434","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Cai and S.-J","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2606.20434","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:39526fdb1c79be4537278e3e710f841663ea47d5eff631ba28a07937c016276a","observation_id":"e91342b9-3415-490e-95b4-1f646a90e870","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.11727","last_updated":"2023-11-10T04:24:20Z","snapshot_observed_at":"2026-08-16T14:51:10.668910Z","submitted_at":"2023-10-18T05:49:26Z","title":"Testing the cosmological principle with the Pantheon+ sample and the region-fitting method","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.11727","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2310.11727","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:0d92107d6ea0bebe1e830c42330e28c97dbba86f7892f4c4ff495a5891df68b6","observation_id":"0e08aefe-333b-4f9e-aac8-d7f70aec9906","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.03624","last_updated":"2020-01-10T19:00:06Z","snapshot_observed_at":"2026-08-15T18:10:27.983089Z","submitted_at":"2020-01-10T19:00:06Z","title":"The Expansion of the Universe is Faster than Expected","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.03624","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2001.03624","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:c2926d9cf2eb2c23415e924c501064b0f380120dd475194ad3978a1d19f067c3","observation_id":"8951cbab-e217-45ed-ba01-afcb38b58bc1","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10625","last_updated":"2019-07-24T18:00:09Z","snapshot_observed_at":"2026-08-15T06:22:52.301428Z","submitted_at":"2019-07-24T18:00:09Z","title":"Tensions between the Early and the Late Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10625","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Verde, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:93c12f60f229b93df673a95114d94d721bc4a9a80b5e2d12ecd492e687b56d3c","observation_id":"9ff142da-5d3a-4e3d-b2f5-286cae1aff82","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11770","last_updated":"2024-10-28T17:53:52Z","snapshot_observed_at":"2026-08-16T13:24:50.358147Z","submitted_at":"2024-08-21T16:47:09Z","title":"JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11770","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2408.11770","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:b9260b8b7c790339492ee686c9ae6a18f613c5add5eededef20ef4f0e22fa564","observation_id":"aa68082f-7c22-4510-81e2-61d2889db764","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.01667","last_updated":"2025-09-01T18:00:01Z","snapshot_observed_at":"2026-08-13T23:28:25.516540Z","submitted_at":"2025-09-01T18:00:01Z","title":"The Perfect Host: JWST Cepheid Observations in a Background-Free SN Ia Host Confirm No Bias in Hubble-Constant Measurements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.01667","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2509.01667","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:3773da852dd2788cb172b3bb01de7ad2d9e1e9fc5c9e2324e292ba53912708ea","observation_id":"d0a66000-d242-4967-92de-a483fdba8e88","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Pantos and L","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:713c808857730fb294348ade4416793a255d03a9e54411086eb569118f16a719","observation_id":"b5faa486-cf12-47f6-9d5c-f0ac6caf6366","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03663","last_updated":"2019-09-16T21:35:34Z","snapshot_observed_at":"2026-08-17T00:55:38.317018Z","submitted_at":"2019-08-10T01:40:10Z","title":"The Hubble Hunter's Guide","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03663","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Knox and M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1908.03663","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:6a47df3354e513ce0c829754783b432c8b195533c1fb4d324c02a49d4045d363","observation_id":"67da3ba2-d794-46d3-9785-804901595118","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.04083","last_updated":"2019-06-11T10:04:20Z","snapshot_observed_at":"2026-08-14T18:01:28.256190Z","submitted_at":"2018-11-09T19:00:00Z","title":"Early Dark Energy Can Resolve The Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.04083","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Poulin, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1811.04083","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:5c9adfafb22e40cf874ebd4a7214fb90d3f081517f49e65680d1742c98131ff6","observation_id":"9e3c14de-cbac-46a9-9ddf-cc540269ceb2","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-08-18T00:05:15.748844Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:6625327efbbf21d6a19a66e6aba44049de92462ba72eb01c470d3326af9a679b","observation_id":"0943c011-10cb-481b-a3c7-1394cd64a8dd","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.15295","last_updated":"2024-09-27T16:01:00Z","snapshot_observed_at":"2026-08-16T14:57:21.583122Z","submitted_at":"2023-09-26T22:20:57Z","title":"Scaling solutions as Early Dark Energy resolutions to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.15295","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2309.15295","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:98ff386fd63e7dcc127a1e9bf24ca2eca57f6569e233e6e6b357a08842139613","observation_id":"00f77fcc-3658-43ac-a028-26c5d4d0fbca","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.05843","last_updated":"2024-05-16T07:49:35Z","snapshot_observed_at":"2026-08-16T13:54:00.237763Z","submitted_at":"2024-05-09T15:27:05Z","title":"Alleviating $H_0$ and $S_8$ Tensions Simultaneously in K-essence Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.05843","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2405.05843","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:64c65a4db2de384da981024349654e76d0122c1a71118a74764f0ca5f50f646b","observation_id":"92344e34-56c3-456a-a167-da47bedaefcf","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.07179","last_updated":"2025-02-13T12:14:51Z","snapshot_observed_at":"2026-08-16T13:44:12.684454Z","submitted_at":"2024-06-11T11:41:41Z","title":"Comprehensive Study of $k$-essence Model: Dynamical System Analysis and Observational Constraints from Latest Type Ia Supernova and BAO Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.07179","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Hussain, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2406.07179","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:83c8dc0a8a9cbb26fc2f4ae83991297b12b42d4a9fe5354ec01bc10c35bb1ce5","observation_id":"3f57f09b-adec-47a4-aa52-ba134063a3ac","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0601544","last_updated":"2006-06-30T13:04:02Z","snapshot_observed_at":"2026-07-07T00:57:52.135465Z","submitted_at":"2006-01-24T17:57:19Z","title":"Early Dark Energy Cosmologies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0601544","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Doran and G","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/0601544","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:6189351d4a4c0e4732bbf4ac6c85a0b309f188f2f12d2d98a769d9cd4ba60910","observation_id":"2daa7168-7819-47a4-9d99-b3401668d95e","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.10739","last_updated":"2021-02-22T15:07:04Z","snapshot_observed_at":"2026-08-13T16:05:35.767229Z","submitted_at":"2019-10-23T18:00:15Z","title":"New Early Dark Energy","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.10739","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Niedermann and M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1910.10739","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:67d26eb308a54c6d5f657a8a693d24b00604ed485af8438cdb1dfbe3d6eff995","observation_id":"deaad118-66cc-4170-97b0-3f9a87b12ef8","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01016","last_updated":"2023-10-07T21:58:58Z","snapshot_observed_at":"2026-08-15T13:42:40.528250Z","submitted_at":"2019-04-01T18:00:00Z","title":"Rock 'n' Roll Solutions to the Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.01016","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Agrawal, F.-Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1904.01016","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:3ecaaceb182cb4b8a8d18f32ce9bd2d375c66e9f49fe174d1f50f4b83b5178e1","observation_id":"fe216736-3aa9-4129-ba8b-37af4767f951","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.07355","last_updated":"2020-07-15T19:00:55Z","snapshot_observed_at":"2026-08-13T23:15:14.344746Z","submitted_at":"2020-03-16T17:59:03Z","title":"Early Dark Energy Does Not Restore Cosmological Concordance","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.07355","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2003.07355","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:8a521824002636ea73eece1c475c49a4972559294e0baeaae7406addaaa012a2","observation_id":"8c1094da-ea96-40af-85ed-6a5cf0dc91b2","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.08252","last_updated":"2018-08-30T08:08:21Z","snapshot_observed_at":"2026-08-14T19:12:49.050661Z","submitted_at":"2018-05-21T18:40:03Z","title":"Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.08252","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1805.08252","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:385233bec84687a5cd67a7ac921d5980b9fd17be5f7590cd4f567ae6fcdf1c20","observation_id":"42913d81-5b3a-45a9-b92f-a2bbca26e9aa","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.04716","last_updated":"2019-04-01T07:53:29Z","snapshot_observed_at":"2026-08-14T19:16:06.534258Z","submitted_at":"2018-05-12T13:01:41Z","title":"Are $H_0$ and $\\sigma_8$ tensions generic to present cosmological data?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.04716","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Bhattacharyya, U","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1805.04716","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:93e0a28fe35fc8cbe071bb281469c29d243bbf321fd184fa607fa6e49741944c","observation_id":"24776d1a-36c8-46b1-865f-d268edef0240","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04865","last_updated":"2019-07-14T11:54:15Z","snapshot_observed_at":"2026-08-14T17:03:37.414748Z","submitted_at":"2019-03-12T12:21:21Z","title":"Dark sector interaction: a remedy of the tensions between CMB and LSS data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04865","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Kumar, R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1903.04865","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:c2484835ccffd0c6004dcc839912621b5b5f46576240655daf2750fa6fdac86b","observation_id":"97ed8656-c255-4363-b25c-fd6f25a2090d","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.09853","last_updated":"2020-02-13T10:31:43Z","snapshot_observed_at":"2026-08-11T07:44:09.092665Z","submitted_at":"2019-10-22T09:23:34Z","title":"Non-minimal dark sector physics and cosmological tensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.09853","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Di Valentino, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1910.09853","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:d596e50540b984378497f9797e633b22253aa98cbbe6068490466ba4194ca453","observation_id":"3dd3d377-bbeb-444b-91b8-2789f60006cb","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.02281","last_updated":"2018-05-20T14:45:13Z","snapshot_observed_at":"2026-08-14T19:48:07.747837Z","submitted_at":"2018-02-07T01:50:42Z","title":"Structure formation in $f(T)$ gravity and a solution for $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.02281","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1802.02281","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:c509776002906127a4365723ca4d507a786b021fd420366d7bae845430180f17","observation_id":"1876a608-d1c5-432e-9e7e-acc0b3e41f17","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.10328","last_updated":"2020-06-02T09:26:16Z","snapshot_observed_at":"2026-08-13T08:21:13.293467Z","submitted_at":"2019-09-20T13:50:46Z","title":"Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.10328","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Escamilla-Rivera and J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1909.10328","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:4f73429f9ea6dcc2c0d23f47fbe088e7ac0820c08462c23b03d29c9cf125264a","observation_id":"dbf031e8-4938-42a4-934f-d901a93860a8","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.03957","last_updated":"2021-03-17T12:59:41Z","snapshot_observed_at":"2026-08-16T19:07:24.409606Z","submitted_at":"2020-11-08T11:26:44Z","title":"Analyzing the $H_0$ tension in $F(R)$ gravity models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.03957","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2011.03957","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:dddd4000733990c48862af74b39ce435370b29673bc385cec95cb196bd9b7030","observation_id":"92792f3c-ae2b-4cbc-b3bd-5f6fedbfa55e","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.12934","last_updated":"2021-01-19T07:18:54Z","snapshot_observed_at":"2026-08-16T19:03:15.723868Z","submitted_at":"2020-11-25T18:36:34Z","title":"Early modified gravity in light of the $H_0$ tension and LSS data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.12934","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Braglia, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2011.12934","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:2cd21239aba6c22276d87b84fb008a706d91ebd6cb583277487bcc31c98e9a82","observation_id":"dd31d541-94c6-4e55-a54b-9fecce8b9664","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.10879","last_updated":"2022-04-04T13:08:47Z","snapshot_observed_at":"2026-08-18T00:19:55.354129Z","submitted_at":"2020-12-20T10:07:15Z","title":"Possible Resolution of the Hubble Tension with Weyl Invariant Gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.10879","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Shimon, Possible resolution of the Hubble ten- sion with Weyl invariant gravity, JCAP04(04), 048, arXiv:2012.10879 [astro-ph.CO]","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2012.10879","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:f140d9ffa996f9009123fa27281abf6a2491c5115916e31fefa08bb94cb8d8dd","observation_id":"3f1b8d2a-e8cd-4f9d-b80f-cb4b7e52c955","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.12041","last_updated":"2022-11-22T06:24:13Z","snapshot_observed_at":"2026-08-16T16:14:18.162825Z","submitted_at":"2022-11-22T06:24:13Z","title":"Generic modification of gravity, late time acceleration and Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.12041","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2211.12041","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:d2f15b5e52db1603c64148bb058f7be9b3e4bda8a18003b7de85648f103532b8","observation_id":"d3efac26-8bfe-4a4b-abbf-6b1732662086","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06328","last_updated":"2023-06-16T12:10:37Z","snapshot_observed_at":"2026-08-16T16:02:14.777990Z","submitted_at":"2023-01-16T09:41:20Z","title":"$H_0$ Tension in Torsion-based Modified Gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06328","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Mandal, O","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2301.06328","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:88b292fc8a7c11f4390f31fa508f59fbf5935ccc4bafcfe336db87e1643d9160","observation_id":"745db124-33cd-4a87-b1c3-6b010aea53d4","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.16044","last_updated":"2023-08-30T14:06:37Z","snapshot_observed_at":"2026-08-16T15:04:35.943475Z","submitted_at":"2023-08-30T14:06:37Z","title":"Alleviating $H_0$ tension in scalar-tensor and bi-scalar-tensor theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.16044","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Petronikolou and E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2308.16044","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:e6d0f94672272f9a611862b2ecbb34ff455f6636b02cb769319b051ee07eed7a","observation_id":"4fd5ff01-b156-4f74-8f01-e763b79fc71b","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:f4c57907183cad165713c55d75e8da38d3cf3735c660e0e4f1c88878c18da5f4","observation_id":"4f2c9b63-769d-4a46-9001-01b751c3c79f","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.20107","last_updated":"2025-08-13T10:37:56Z","snapshot_observed_at":"2026-08-14T11:35:27.713122Z","submitted_at":"2025-08-13T10:37:56Z","title":"Testing $f(T)$ Gravity with Cosmological Observations: Confronting the Hubble Tension and Implications for the Late-Time Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.20107","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Verma, A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2508.20107","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:468dbbb0af55392221b2125928d79c074fb255c20617dd716eb28e1bc5862ea2","observation_id":"fa7f8077-aa7d-46a5-8652-3c521865adab","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.08275","last_updated":"2020-01-12T15:03:10Z","snapshot_observed_at":"2026-08-16T18:21:16.865294Z","submitted_at":"2019-06-19T18:00:25Z","title":"A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.08275","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Li and A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1906.08275","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:13dec1c56a9ebc79a01ec6e7cdc1f9510b456d6f24374b6ce72f07192c7e1827","observation_id":"7986744a-f329-4f7d-bcb0-b66ac015a8bc","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.12587","last_updated":"2021-03-29T08:08:31Z","snapshot_observed_at":"2026-08-15T04:10:44.436736Z","submitted_at":"2020-05-26T09:14:59Z","title":"Dark Energy with Phantom Crossing and the $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.12587","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Di Valentino, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2005.12587","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:ba5a2e7243de9ab641c858e5ec789b161f2502c48925bd89a71ccc8c181a43c6","observation_id":"508f3a0f-cfc8-407e-a014-2b92bee5b00d","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.03815","last_updated":"2021-09-09T18:46:54Z","snapshot_observed_at":"2026-08-16T18:40:55.746279Z","submitted_at":"2021-03-05T17:28:12Z","title":"Generalized Emergent Dark Energy Model and the Hubble Constant Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.03815","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2103.03815","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:64966ef501996410c6d4e7e280fc6b0cd5974e640c9ce6800247cb08fa53e1e1","observation_id":"cee567d3-06db-49e2-999c-7fed51d5b07b","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Adi, Lowering the Horizon on Dark Energy: A Late-Time Response to Early Solutions for the Hubble Tension, arXiv preprint arXiv:2509.12331 (2025), arXiv:2509.12331 [astro-ph.CO]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:b8e47a7d718c538c023b1588e749f9e1fa7fea849e4ae1be412d253ac139bdb2","observation_id":"e92c0f19-9bc8-4ac4-afdd-91a4a04cc4c8","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2512.07281","last_updated":"2026-06-24T11:03:08Z","snapshot_observed_at":"2026-08-15T11:40:36.328100Z","submitted_at":"2025-12-08T08:20:26Z","title":"Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2512.07281","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Zhang, T","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2512.07281","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:b4e072d2c5f9e15731ae348a6899fda51fa4a7c09a645e9b7751ce25c2178330","observation_id":"524dd441-4ba2-48c2-a4ac-aaab4f3ceae9","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.10868","last_updated":"2020-04-22T21:22:49Z","snapshot_observed_at":"2026-08-09T15:23:02.533059Z","submitted_at":"2020-04-22T21:22:49Z","title":"Self-interacting neutrinos: solution to Hubble tension versus experimental constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.10868","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2004.10868","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:e6991ebaf39e8ee60ed272ee7a621b79209416b9617224ee7496a13e6dfa2dcb","observation_id":"318e996b-bfa1-4557-9991-5d173d225a78","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.03990","last_updated":"2022-04-19T02:07:30Z","snapshot_observed_at":"2026-08-16T17:50:54.296645Z","submitted_at":"2021-10-08T09:20:00Z","title":"Minimal dark energy: key to sterile neutrino and Hubble constant tensions?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.03990","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Di Valentino, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2110.03990","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:aecd855a6b74403f790e3084b5f1bc97146a75758fbcdb471a37a6a99d9d611b","observation_id":"deedce87-8729-461c-9fcb-09d30fc98146","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Yarahmadi, A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:700adf8502145e093f59e8739b71ee9eefa8b35dd456900cfb9495751edc2fed","observation_id":"3447f212-90a6-480f-8b7e-2437334116cc","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Armendariz-Picon, T","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:d4b1dc7c57a8a568a3341957729d92c1468e89a79fc8e9af1f11f4d661621dc1","observation_id":"9d9e3a8c-5be9-4329-a015-96bbdf290c27","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Armendariz-Picon, V","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:db6d50501a56a00609b40ed7711756a0ad73962fd28c0fd599f7fccb32c287d8","observation_id":"f1347454-2d1a-4cf0-b043-8231e64997d9","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9912463","last_updated":"2000-01-29T04:38:58Z","snapshot_observed_at":"2026-08-05T23:35:03.953059Z","submitted_at":"1999-12-22T12:12:41Z","title":"Kinetically Driven Quintessence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9912463","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Chiba, T","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/9912463","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:79831ac7dfb9afef02a8765d8c403bdc1aa6cfd0f7dc2100c0eaef795847bc37","observation_id":"ec6ecaa1-b654-4363-8243-7df5f7388ad0","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0006373","last_updated":"2000-06-27T00:01:38Z","snapshot_observed_at":"2026-08-03T23:32:34.694893Z","submitted_at":"2000-06-27T00:01:38Z","title":"Essentials of k-essence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0006373","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Armendariz-Picon, V","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/0006373","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:eca6de9401a03760b2b0f69cee108aba6807bd5946037b90043a2532c6af35b7","observation_id":"75bbab0b-ab72-4c29-bed0-f1f48c48ab0e","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0405054","last_updated":"2004-07-26T13:02:13Z","snapshot_observed_at":"2026-07-07T04:50:31.853301Z","submitted_at":"2004-05-07T11:26:23Z","title":"Dilatonic ghost condensate as dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0405054","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Piazza and S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/hep-th/0405054","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:c614b91bca1c15c8a5ed829c20b07f28c0a5e38a0cbe932849658a49caa5e7fd","observation_id":"175e28b6-c124-4ed6-b535-cf75e5710bb7","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Amendola and S","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:ca47e3af22def9b9262ebd2a3144426aba0f8e94e63496e1f60445732363602e","observation_id":"ead032e8-f8e8-4339-acef-6d14262038c8","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.20989","last_updated":"2026-04-22T18:21:13Z","snapshot_observed_at":"2026-08-13T20:08:31.874747Z","submitted_at":"2026-04-22T18:21:13Z","title":"Relativistic effects in k-essence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.20989","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Duniya, I","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2604.20989","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:c87dd5adb2606c178a2cf82fea137c6706b5292a90fc732f3335780b0f73055b","observation_id":"43cab972-fb67-4ab8-8f1a-d98af1e3a4ee","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0212198","last_updated":"2003-03-05T07:02:00Z","snapshot_observed_at":"2026-07-07T00:30:10.687769Z","submitted_at":"2002-12-09T09:45:43Z","title":"Cosmology with tachyon field as dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0212198","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/0212198","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:df1a7d4d5dd8e2ac377acb2fce8974b30bfb7ed90c99f0c017c1b411f049fa69","observation_id":"bab8dbeb-5de2-46c9-972f-249126ddb031","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0311613","last_updated":"2004-04-16T23:41:15Z","snapshot_observed_at":"2026-08-03T15:34:31.124861Z","submitted_at":"2003-11-27T21:19:43Z","title":"Extended tachyon field, Chaplygin gas and solvable k-essence cosmologies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0311613","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/0311613","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:e7e72020e7249b5a791e42e80d9175eccb393d0f0c15c8c5c7a5f78f18840f2f","observation_id":"8c9e915a-18be-40d2-96f5-1bce2ce3e08e","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:5b59c636d197e77db0602d353f52b71ee55e0eddd658c593145d91b2bf1a7239","observation_id":"dfd96a9f-9054-464a-8a7d-dcbc3a4b2db7","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9905040","last_updated":"1999-10-12T09:02:54Z","snapshot_observed_at":"2026-07-07T01:25:56.760989Z","submitted_at":"1999-05-05T13:40:56Z","title":"Quintessence and Supergravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9905040","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Brax and J","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/9905040","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:b67971f3873216bcf9ad3a6958a3352e07b7fc326a18b4ae52c59aa006d18f7f","observation_id":"977cca44-cb16-4323-92d0-b85ce743c27f","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9910214","last_updated":"2001-01-16T16:40:51Z","snapshot_observed_at":"2026-08-06T23:58:50.642721Z","submitted_at":"1999-10-12T16:47:15Z","title":"Quintessence arising from exponential potentials","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9910214","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Barreiro, E","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/9910214","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:e854cd9ec5a52fa7e304c21a6a14468d0b6c102275924b952856b7fb7f3c013a","observation_id":"322d5150-1694-4945-a04b-5dd1a43f0f79","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.1961","last_updated":"2013-10-05T08:56:41Z","snapshot_observed_at":"2026-08-15T00:22:22.422604Z","submitted_at":"2013-04-07T06:21:37Z","title":"Quintessence: A Review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.1961","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Tsujikawa, Quintessence: A Review, Class","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1304.1961","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:878aba229d81111203fd7a94548fc647051be7f88ea0d6f5e98763eab883c87c","observation_id":"86aa2eab-a5b3-4420-a40f-0805af014939","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.05724","last_updated":"2018-08-17T01:37:03Z","snapshot_observed_at":"2026-08-15T09:32:46.755362Z","submitted_at":"2018-08-17T01:37:03Z","title":"Distance Priors from Planck Final Release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.05724","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Chen, Q.-G","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1808.05724","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:1a8759dc786939edc920b41960711a0693b22dc69b9c1bb1ede4f00e26fb2762","observation_id":"03dc0afe-776f-42f5-be76-33185b8bed8c","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03863","last_updated":"2022-02-07T19:00:01Z","snapshot_observed_at":"2026-07-06T12:16:15.735863Z","submitted_at":"2021-12-07T17:57:21Z","title":"The Pantheon+ Analysis: The Full Dataset and Light-Curve Release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03863","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Scolnicet al., The Pantheon+ Analysis: The Full Data Set and Light-curve Release, Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2112.03863","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:0dcecaaa7d8a96408f2e3d7ed735b98a65740a07cbb454ed4e6c264609cbd7e4","observation_id":"5c8bfa40-5fc9-47be-90e8-9fcc2bd9ebcb","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04077","last_updated":"2022-11-14T21:28:25Z","snapshot_observed_at":"2026-08-01T22:04:41.273741Z","submitted_at":"2022-02-08T19:00:00Z","title":"The Pantheon+ Analysis: Cosmological Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04077","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Broutet al., The Pantheon+ Analysis: Cosmo- logical Constraints, Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2202.04077","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:79752473dab36941720a1b5cc7bdfc702029a4c581c3c5b47fb686a0d5b5d0a2","observation_id":"9cfb048a-01f7-4cc8-91a2-a531b9b89308","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"com/PantheonPlusSH0ES/DataRelease","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:008e248289f3540606170a5b3f44d39a13889117c6b80aa5473fc0930d1f15c3","observation_id":"c5f5185c-4b20-4d86-9119-28e23574f479","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.12098","last_updated":"2025-06-20T17:34:15Z","snapshot_observed_at":"2026-08-14T04:04:21.819442Z","submitted_at":"2023-11-20T19:00:01Z","title":"Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.12098","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Rubinet al., Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework, Astrophys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2311.12098","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:9d02c07902edf57ef5e4f036c799e17b70de04dfea836d2e386546f64b6dd3b3","observation_id":"95221956-36d7-45e0-86c9-782ff6aecd9e","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.02929","last_updated":"2025-07-20T07:40:37Z","snapshot_observed_at":"2026-08-16T23:26:10.062416Z","submitted_at":"2024-01-05T18:14:39Z","title":"The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.02929","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2401.02929","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:c69abada10954ef8fc9191af06ad13b22f566781e9e6e001956cd0a1094625ba","observation_id":"1d5bce92-f473-4c62-b5b4-fcd4c45c90f1","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.01024","last_updated":"2023-01-26T18:23:17Z","snapshot_observed_at":"2026-08-16T16:04:43.393826Z","submitted_at":"2023-01-03T09:54:49Z","title":"On the homogeneity of SnIa absolute magnitude in the Pantheon+ sample","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.01024","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Perivolaropoulos and F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2301.01024","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:880d34880787cf20061756889027aefa8300b9a142d4e0a33a611874289f72f6","observation_id":"349e5fd8-a198-41ff-bd2f-280f95ef08e0","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.07425","last_updated":"2018-11-23T17:29:48Z","snapshot_observed_at":"2026-08-15T02:05:20.617689Z","submitted_at":"2018-11-18T23:36:42Z","title":"Robust and model-independent cosmological constraints from distance measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.07425","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Zhai and Y","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1811.07425","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:a9760bffceebb7bb9d6f11d7ee7efea2a6e6f60ab5c53956b16571ff74a31029","observation_id":"1c7bbd16-c45e-43ad-ace5-6ae9976a2937","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.17792","last_updated":"2025-03-08T08:41:48Z","snapshot_observed_at":"2026-08-16T12:55:31.484092Z","submitted_at":"2025-02-25T02:50:16Z","title":"Cosmological constraints on two vacuum decay models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.17792","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2502.17792","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:b7ddaa7a34a22fe28ecf9951c412ee86296db50641914bda8c6429a47dad2512","observation_id":"b0dc5989-30b4-4fb3-b2bc-d2ac4172e47e","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Yang, Constraining deviations fromΛCDM in the Hubble expansion rate, Eur","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:22057c368e55ddc0396fd050eab3df8a68eccc4c5ff9c494e7e59f3406daae61","observation_id":"7aacdf3d-a528-4bf0-be3f-44256b7edca9","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.4514","last_updated":"2013-08-29T16:18:47Z","snapshot_observed_at":"2026-08-16T07:53:48.404600Z","submitted_at":"2013-04-16T16:38:50Z","title":"Distance Priors from Planck and Dark Energy Constraints from Current Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.4514","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Wang and S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1304.4514","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:3f72217d9ce1de1ceafd46c137a05880da7cdb68a1feac47a6ae48640b05470b","observation_id":"2dbbe2ec-fd92-461f-a238-7247d08ed18d","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.0223","last_updated":"2015-07-03T14:08:48Z","snapshot_observed_at":"2026-08-14T23:21:19.168238Z","submitted_at":"2014-08-31T14:19:21Z","title":"Updated reduced CMB data and constraints on cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.0223","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Cai, Z.-K","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1409.0223","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:15c5fef15cb914354367c3c168983d0e26eab13d237696a394dfc3eb880f4c63","observation_id":"0fab67fe-b5e3-41ff-abc6-7503e1e015b4","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9510117","last_updated":"1996-04-19T18:52:38Z","snapshot_observed_at":"2026-07-07T01:12:03.384465Z","submitted_at":"1995-10-23T16:35:10Z","title":"Small Scale Cosmological Perturbations: An Analytic Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9510117","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Hu and N","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/9510117","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:61dd66466a98dcd249dcd251be76173355afefeef564e53055a2a117195dea11","observation_id":"dc571918-497f-4326-a751-3298fc8dc94c","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:1802f13f54b4c586c04ed8bd292f4a4583995c1accb031d9dc076ee0909a96a8","observation_id":"b59b98a0-b274-4346-ae66-573e3df272cb","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Abdul Karimet al.(DESI), DESI DR2 results","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:5c79d9391f91396ed65d6176a12c322bcb5208e6c535fee4249935999081ca81","observation_id":"a2362090-bb34-4c88-af45-cbd7d52f9fed","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9709112","last_updated":"1997-09-12T00:10:17Z","snapshot_observed_at":"2026-07-07T01:18:17.177186Z","submitted_at":"1997-09-12T00:10:17Z","title":"Baryonic Features in the Matter Transfer Function","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9709112","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/astro-ph/9709112","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:d5099c626593d629fe380756f9e38e2d86b87e5145c51599c65085adc5bc5550","observation_id":"5d2200e8-40e3-48bc-a648-062cd39fafba","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03437","last_updated":"2018-03-11T22:31:08Z","snapshot_observed_at":"2026-08-14T20:15:15.991128Z","submitted_at":"2017-11-09T15:55:12Z","title":"Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially-Flat $\\Lambda$cdm Model, The Deceleration-Acceleration Transition Redshift, and Spatial Curvature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03437","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1711.03437","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:69161384787772c01114774d34bc281b1840de8f5285b9173c66bc7d15a18b3e","observation_id":"0677c735-1ac4-4310-84c8-f4f1487232d0","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.3609","last_updated":"2013-02-05T14:57:11Z","snapshot_observed_at":"2026-08-15T04:22:12.360214Z","submitted_at":"2012-01-17T20:19:31Z","title":"Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.3609","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1201.3609","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:7520bc70bd6295bb82af91ea22dd767e9b23f4da553520661012286b48042095","observation_id":"fa42c337-3dc1-4937-97f6-d1e3774bc061","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.1801","last_updated":"2014-12-15T17:04:34Z","snapshot_observed_at":"2026-08-14T23:38:23.907730Z","submitted_at":"2014-04-07T14:43:36Z","title":"Baryon Acoustic Oscillations in the Ly{\\alpha} forest of BOSS DR11 quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.1801","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Delubacet al.(BOSS), Baryon acoustic oscillations in the Lyαforest of BOSS DR11 quasars, Astron","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1404.1801","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:38a7728780ddbcbc00fe7597f8ac91f5b8a1d6a81c7a2864883f03f3095ec0f7","observation_id":"0e9406fd-ea83-4731-a4df-b59e0ec99b33","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03155","last_updated":"2016-07-11T20:29:52Z","snapshot_observed_at":"2026-08-14T21:48:51.809084Z","submitted_at":"2016-07-11T20:29:52Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03155","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Alamet al.(BOSS), The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectro- scopic Survey: cosmological analysis of the DR12 galaxy sample, Mon","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1607.03155","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:ab1703ba04cf9f21e1e25ec8a43f9d6b39dc939ea416be18dee1dc0e6396aad5","observation_id":"5e56662b-a1bd-4382-9d5e-1ce67b980bf9","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.5226","last_updated":"2013-06-04T19:07:35Z","snapshot_observed_at":"2026-08-15T00:34:53.864487Z","submitted_at":"2012-12-20T20:24:52Z","title":"Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.5226","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Hinshawet al.(WMAP), Nine-Year Wilkinson Mi- crowave Anisotropy Probe (WMAP) Observations: Cos- mological Parameter Results, Astrophys","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/1212.5226","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:831ae25ef1b5bc6b95fdb3b0e292dda772f7617ee9750e5ed396650e0f28ebbb","observation_id":"c2c1b340-f53a-417f-828d-9bf67e59698b","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.07288","last_updated":"2020-12-03T21:07:24Z","snapshot_observed_at":"2026-08-10T12:34:10.737722Z","submitted_at":"2020-07-14T18:38:20Z","title":"The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.07288","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Aiolaet al.(ACT), The Atacama Cosmology Tele- scope: DR4 Maps and Cosmological Parameters, JCAP 12, 047, arXiv:2007.07288 [astro-ph.CO]","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2007.07288","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:484ffe29e1877b91ed964ecebc8bf1328d391501abc871f8dcf743249987ef5c","observation_id":"1eed19b8-80e2-4c8a-af25-451fde680f65","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.01684","last_updated":"2021-01-05T18:05:08Z","snapshot_observed_at":"2026-08-17T10:43:33.063575Z","submitted_at":"2021-01-05T18:05:08Z","title":"Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.01684","snapshot_observed_at":"2026-07-12T01:30:43.080456Z","title":"Dutcheret al.(SPT-3G), Measurements of the E- mode polarization and temperature-E-mode correlation of the CMB from SPT-3G 2018 data, Phys","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-07-12T01:30:43.080456Z"},"links":{"cited_paper":"/paper/2101.01684","citing_paper":"/paper/2607.03569"},"observation_digest":"sha256:0e68a6bb60971be03f4b29f24e4cd365ccd1fb01db55ab1fea0c1ac3a408df7e","observation_id":"eecec74b-d3c1-4429-b974-5c8b3ba96846","resolution":{"observed_at":"2026-07-12T01:30:43.080456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.03569","last_updated":"2026-07-03T19:18:39Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-05T10:10:25.674240Z","submitted_at":"2026-07-03T19:18:39Z","title":"Hubble tension in k-essence: Evidence for robust tension alleviation"},"reference_resolution":{"displayed":86,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":86,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":86},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 86 of 86 outbound references and 0 inbound Pith citation observations for arXiv:2607.03569."}